File:Rhessi0269 web.jpg

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English: RHESSI Observes 2.2 MeV Line Emission from a Solar Flare. The solar flare at Active Region 10039 on July 23, 2002 exhibits many exceptional high-energy phenomena including the 2.223 MeV neutron capture line and the 511 keV electron-positron (antimatter) annihilation line. In the animation, the RHESSI low-energy channels (12-25 keV) are represented in red and appears predominantly in coronal loops. The high-energy flux appears as blue at the footpoints of the coronal loops. Violet is used to indicate the location and relative intensity of the 2.2 MeV emission.
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Source NASA - National Aeronautics and Space Administration Visible Earth A catalog of NASA images and animations of our home planet Solar Flare 2.2MeV Line Emissions
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  1. Writer William Steigerwald # Visualization Date 2003/06/11 # Scientist Sam Krucker (University of California at Berkeley), Gordon J. Hurford (University of California at Berkeley), Robert Lin (University of California at Berkeley), R. J. Murphy (NRL), G. H. Share (NRL), X.-M. Hua (L-3 Communications Analytics Corporation), David M. Smith (University of California at Berkeley), Richard A. Schwartz (NASA/GSFC), Benzion Kozlovsky (Tel Aviv University).
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Credit: NASA/Goddard Space Flight Center Scientific Visualization Studio

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current21:29, 10 October 2009Thumbnail for version as of 21:29, 10 October 2009320 × 240 (6 KB)Marshallsumter (talk | contribs){{Information |Description={{en|1=RHESSI Observes 2.2 MeV Line Emission from a Solar Flare. The solar flare at Active Region 10039 on July 23, 2002 exhibits many exceptional high-energy phenomena including the 2.223 MeV neutron capture line and the 511 k

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